Formation of Jupiter by nucleated instability
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Typical values of ξ are expected to be in the range 0.1 < ξ < 0.3.
“Simulations indicate that ξ > 0 . 4 are unlikely and that typical values are expected to be in the range of 0 . 1 < ξ < 0 . 3 (Quillen & Trilling 1998; Canup & Ward 2002; Magni & Coradini 2004; Ayliffe & Bate 2009; Ward & Canup 2010).”
From Mass and period limits on the ringed companion transiting the young star J1407 (2015) · cites this paper as Magni & Coradini 2004
For Galilean satellites forming in the Jovian circumplanetary disk after dissipation, smaller values of ξ ~0.1-0.2 are found.
“For the Galilean satellites forming in the Jovian circumplanetary disk after dissipation, smaller values of ξ ∼ 0 . 1 -0 . 2 are found (Canup & Ward 2002; Magni & Coradini 2004; Ward & Canup 2010).”
From Mass and period limits on the ringed companion transiting the young star J1407 (2015) · cites this paper as Magni & Coradini 2004
Simulations indicate that ξ > 0.4 are unlikely.
“Simulations indicate that ξ > 0 . 4 are unlikely and that typical values are expected to be in the range of 0 . 1 < ξ < 0 . 3 (Quillen & Trilling 1998; Canup & Ward 2002; Magni & Coradini 2004; Ayliffe & Bate 2009; Ward & Canup 2010).”
From Mass and period limits on the ringed companion transiting the young star J1407 (2015) · cites this paper as Magni & Coradini 2004
The existence of circumplanetary disks after the dissipation of the protosolar nebular disk has been postulated from formation scenarios for the Galilean satellites.
“The existence of circumplanetary disks after the dissipation of the protosolar (circumstellar) nebular disk has been postulated from formation scenarios for the Galilean satellites (Canup & Ward 2002;Magni & Coradini 2004;Ward & Canup 2010).”
From PLANETARY CONSTRUCTION ZONES IN OCCULTATION: DISCOVERY OF AN EXTRASOLAR RING SYSTEM TRANSITING A YOUNG SUN-LIKE STAR AND FUTURE PROSPECTS FOR DETECTING ECLIPSES BY CIRCUMSECONDARY AND CIRCUMPLANETARY DISKS (2012) · cites this paper as Magni & Coradini 2004
After gas is cleared out of the planetary system, dust in the circumplanetary disk accretes into moons or remains as a ring system within the Roche limit of the planet.
“After the gas is cleared out of the planetary system, dust in the circumplanetary disk then accretes into moons or remains as a ring system within the Roche limit of the planet (Canup & Ward 2002;Magni & Coradini 2004;Ward & Canup 2010).”
From MODELING GIANT EXTRASOLAR RING SYSTEMS IN ECLIPSE AND THE CASE OF J1407B: SCULPTING BY EXOMOONS? (2015) · cites this paper as Magni & Coradini 2004
Cites
Formation of the Galilean Satellites: Conditions of Accretion
Canup, R. M., & Ward, W. R. (2002) · The Astronomical Journal · doi:10.1086/344684 · Cited by 433 · see citing works
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Exploring The Saturn System In The Thermal Infrared: The Composite Infrared Spectrometer
Flasar, F., Kunde, V., Abbas, M., Achterberg, R., Ade, P., Barucci, A., Bézard, B., Bjoraker, G., Brasunas, J., Calcutt, S., et al. (2004) · Space Science Reviews · doi:10.1007/s11214-004-1454-9 · Cited by 313 · see citing works
Self-citationAtmospheric Escape and Evolution of Terrestrial Planets and Satellites
Lammer, H., Kasting, J. F., Chassefière, E., Johnson, R. E., Kulikov, Y. N., & Tian, F. (2008) · Space Science Reviews · doi:10.1007/s11214-008-9413-5 · Cited by 275 · see citing works
“…by avoiding the limitations in Mousis et al. (2002) such as “equilibrium of Saturn’s subnebula during its cooling phase” and neglecting the fact that Saturn accreted gas and gas coupled material during a substantial fraction of the subnebula lifetime (Lubow et al. 1999; Magni and Coradini 2004).”
BackgroundEnrichment in volatiles in the giant planets of the Solar System
Hersant, F., Gautier, D., & Lunine, J. (2004) · Planetary and Space Science · doi:10.1016/j.pss.2003.12.011 · Cited by 149 · see citing works
Mamajek, E. E., Quillen, A. C., Pecaut, M. J., Moolekamp, F., Scott, E. L., Kenworthy, M. A., Cameron, A. C., & Parley, N. R. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/143/3/72 · Cited by 140 · see citing works
“Recent explorations of circumplanetary disks separate the disk evolution into two phases (Alibert et al. 2005; Ward & Canup 2010).”
BackgroundMethodInfluentialMODELING GIANT EXTRASOLAR RING SYSTEMS IN ECLIPSE AND THE CASE OF J1407B: SCULPTING BY EXOMOONS?
Kenworthy, M. A., & Mamajek, E. E. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/800/2/126 · Cited by 123 · see citing works
“After the gas is cleared out of the planetary system, dust in the circumplanetary disk then accretes into moons or remains as a ring system within the Roche limit of the planet (Canup & Ward 2002; Magni & Coradini 2004; Ward & Canup 2010).”
BackgroundCIRCUMPLANETARY DISK FORMATION
Ward, W. R., & Canup, R. M. (2010) · The Astronomical Journal · doi:10.1088/0004-6256/140/5/1168 · Cited by 116 · see citing works
“…has expanded considerably, and recently a new class of models has emerged utilizing a top-down approach that attempts to describe disk generation in the context of giant planet formation and contraction (Canup & Ward 2002, 2006, 2009; Magni & Coradini 2004; Alibert et al. 2005; Sasaki et al. 2010).”
BackgroundTandEM: Titan and Enceladus mission
Coustenis, A., Atreya, S. K., Balint, T., Brown, R. H., Dougherty, M. K., Ferri, F., Fulchignoni, M., Gautier, D., Gowen, R. A., Griffith, C. A., et al. (2008) · Experimental Astronomy · doi:10.1007/s10686-008-9103-z · Cited by 101 · see citing works
Self-citationThe Origin and Evolution of Titan
Lunine, J. I., Choukroun, M. N., Stevenson, D. J., & Tobie, G. (2009) · Springer eBooks · doi:10.1007/978-1-4020-9215-2_3 · Cited by 66 · see citing works
Interpretation of the carbon abundance in Saturn measured by Cassini
Hersant, F., Gautier, D., Tobie, G., & Lunine, J. I. (2008) · Planetary and Space Science · doi:10.1016/j.pss.2008.02.007 · Cited by 68 · see citing works
Formation of Titan in Saturn's subnebula : constraints from Huygens probe measurements
Alibert, Y., & Mousis, O. (2007) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20066402 · Cited by 54 · see citing works
The dependence of protoplanet migration rates on co-orbital torques
D'Angelo, G., Bate, M., & Lubow, S. (2004) · doi:10.1111/j.1365-2966.2005.08866.x · Cited by 48
“…been found recently (Rice & Armitage 2003; Alibert, Mordasini & Benz 2004) that the effects of accretion and migration of a planetary core can significantly reduce the time needed by the core to reach the mass necessary for the nucleated instability to occur (Wuchterl 1991b; Magni & Coradini 2004).”
BackgroundFormation and Composition of Planetesimals
Gautier, D., & Hersant, F. (2005) · doi:10.1007/s11214-005-1946-2 · Cited by 48
LAPLACE: A mission to Europa and the Jupiter System for ESA’s Cosmic Vision Programme
Blanc, M., Alibert, Y., André, N., Atreya, S., Beebe, R., Benz, W., Bolton, S., Coradini, A., Coustenis, A., Dehant, V., et al. (2009) · Experimental Astronomy · doi:10.1007/s10686-008-9127-4 · Cited by 47 · see citing works
“When a critical mass is reached, the cores start to capture ever increasing quantities of nebular gas, leading to a phase of gas accretion where the planets grow to their final masses [50].”
BackgroundSelf-citationModeling the Jovian subnebula: I. Thermodynamic conditions and migration of proto-satellites.
Alibert, Y., Mousis, O. J., & Benz, W. (2005) · HAL · doi:10.1051/0004-6361:20052841 · Cited by 36 · see citing works
“The outer radius of the subnebula is taken equal to 150 RJ ∼ 1/5×RHill, a value close to the one calculated by Magni & Coradini (2004) using a 3D hydrodynamical model of the end of Jupiter’s formation.”
MethodWater, heat, bombardment: The evolution and current state of (2) Pallas
Schmidt, B. E., & Castillo-Rogez, J. C. (2011) · Icarus · doi:10.1016/j.icarus.2011.11.019 · Cited by 17 · see citing works
“The timescales and the other parameters, on which our modeling was based, were derived from the results of hydrodynamical simulations described in Magni & Coradini (2004) and Coradini, Magni & Turrini (2010) and consistently with the findings of Lissauer et al. (2009).”
MethodSelf-citationCeres water regime: surface temperature, water sublimation and transient exo(atmo)sphere
Formisano, M., Sanctis, M. D. D., Magni, G., Federico, C., & Capria, M. T. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2344 · Cited by 40 · see citing works
Self-citationMass and period limits on the ringed companion transiting the young star J1407
Kenworthy, M. A., Lacour, S., Kraus, A., Triaud, A. H. M. J., Mamajek, E. E., Scott, E. L., Ségransan, D., Ireland, M., Hambsch, F.-J., Reichart, D. E., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2067 · Cited by 36 · see citing works
“For the Galilean satellites forming in the Jovian circumplanetary disk after dissipation, smaller values of ξ ∼ 0.1 − 0.2 are found (Canup & Ward 2002; Magni & Coradini 2004; Ward & Canup 2010).”
BackgroundMethodInfluentialConstraints from deuterium on the formation of icy bodies in the Jovian system and beyond
Horner, J., Mousis, O., Alibert, Y., Lunine, J., & Blanc, M. (2008) · Planetary and Space Science · doi:10.1016/j.pss.2008.04.010 · Cited by 33 · see citing works
“Matter flowing from the Solar nebula to the forming planet forms a circum-planetary disk, known as a subnebula, in which regular satellites are believed to form (Lubow et al., 1999; Magni and Coradini, 2004).”
BackgroundMethodJOVIAN EARLY BOMBARDMENT: PLANETESIMAL EROSION IN THE INNER ASTEROID BELT
Turrini, D., Coradini, A., & Magni, G. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/750/1/8 · Cited by 34 · see citing works
“The e-folding time τg = 5 × 103 years is derived from the hydrodynamical simulations described in Magni & Coradini (2004), Lissauer et al. (2009), and Coradini et al. (2010).”
MethodSelf-citationFrom Gas to Satellitesimals: Disk Formation and Evolution
Coradini, A., Magni, G., & Turrini, D. (2009) · Space Science Reviews · doi:10.1007/s11214-009-9611-9 · Cited by 28 · see citing works
“Theoretical works have modeled the process of gas accretion invoking hydrodynamic instability (Magni & Coradini, 2004) or quasi-hydrostatic, irradiation-driven compression (Lissauer et al., 2009).”
BackgroundMethodInfluentialSelf-citationJIRAM, the Image Spectrometer in the Near Infrared on Board the Juno Mission to Jupiter
Adriani, A., Coradini, A., Filacchione, G., Lunine, J., Bini, A., Pasqui, C., Calamai, L., Colosimo, F., Dinelli, B. M., Grassi, D., et al. (2008) · Astrobiology · doi:10.1089/ast.2007.0167 · Cited by 21
“Juno’s microwave sounder will address a key issue for giant planet formation, which is the deep water abundance— that is, the value well below 10 bar (Magni and Coradini, 2004; see references in Lunine et al ., 2004).”
Self-citationGaulme, P., Mosser, B., Schmider, F., Guillot, T., & Jackiewicz, J. (2014) · doi:10.1017/cbo9781107300668.017 · Cited by 19
Lazzoni, C., Zurlo, A., Desidera, S., Mesa, D., Fontanive, C., Bonavita, M., Ertel, S., Rice, K., Vigan, A., Boccaletti, A., et al. (2020) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201937290 · Cited by 18 · see citing works
“However, we would expect the mass of a disk surrounding a substellar object to scale with the mass of the companion itself (Magni & Coradini 2004); satellites and ring systems should also follow such trends (Ward & Canup 2010).”
BackgroundMentel, R. T., Kenworthy, M. A., Cameron, D. A., Scott, E. L., Mellon, S. N., Hudec, R., Birkby, J. L., Mamajek, E. E., Schrimpf, A., Reichart, D. E., et al. (2018) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201834004 · Cited by 14 · see citing works
“The circumplanetary disk subsequently accretes onto the planet or into moons (Canup & Ward 2002; Magni & Coradini 2004; Ward & Canup 2010).”
BackgroundSpectral studies of asteroids 21 lutetia and 4 vesta as objects of space missions
Busarev, V. (2010) · doi:10.1134/s0038094610060043 · Cited by 9
Osborn, H., Kenworthy, M., Rodriguez, J., de Mooij, E. J. W., Kennedy, G., Relles, H., Gomez, E., Hippke, M., Banfi, M., Barbieri, L., et al. (2019) · Monthly notices of the Royal Astronomical Society · doi:10.1093/mnras/stz283 · Cited by 8 · see citing works
Formation and early evolution of Io
McKinnon, W. (2007) · Springer eBooks · doi:10.1007/978-3-540-48841-5_4 · Cited by 6 · see citing works
Saturn Satellites as Seen by Cassini Mission
Coradini, A., Capaccioni, F., Cerroni, P., Filacchione, G., Magni, G., Orosei, R., Tosi, F., & Turrini, D. (2009) · doi:10.1007/s11038-009-9334-7 · Cited by 5
Self-citationModels of the protosatellite disk of Saturn: Conditions for Titan’s formation
Makalkin, A. B., & Dorofeeva, V. (2006) · Solar System Research · doi:10.1134/s0038094606060013 · Cited by 4 · see citing works
The role of Fischer-Tropsch catalysis in Jovian subnebular chemistry
Mousis, O., Alibert, Y., Sekine, Y., Sugita, S., & Matsui, T. (2006) · doi:10.1051/0004-6361:20064947 · Cited by 3
“The initial accretion rate and radius of the subdisk have been constrained by models of Jupiter’s formation (Alibert et al. 2005b; Magni & Coradini 2004).”
BackgroundMethodInfluentialCratering records on Vesta and Ceres: a probe in the history of Solar System?
Turrini, D., Magni, G., & Coradini, A. (2010) · doi:10.1051/eas/1041033 · Cited by 1
Self-citation
- Authors
- Magni, G., & Coradini, A.
- Affiliations
- National Institute for Astrophysics (IT)
- Corresponding author
- Magni, Gianfranco
- Venue
- Planetary and Space Science
- Publisher
- Elsevier BV
- Published
- 2004-04
- Volume
- 52
- Issue
- 5-6
- Pages
- 343-360
- ISSN
- 0032-0633 (ISSN-L)
- OpenAlex
- W2036435441
- Cited by
- 44
- References
- 0
- Citations by year
- 2023: 1 · 2020: 2 · 2019: 1 · 2018: 3 · 2015: 2 · 2014: 1 · 2012: 2
- FWCI
- 2.36
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Planetary and Space Science (publishedVersion)
- Funders
- Agenzia Spaziale Italiana (IR 220/02)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- Jupiter formation, giant planet formation, protoplanetary disks, angular momentum transport, exoplanets
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